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High-Resolution Infrared Spectroscopy of Protoplanetary Disks

  • Carr J
Springer-Verlag, (2006), 203-213
DOI: 10.1007/10995082_31
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Abstract

High-resolution spectroscopy at near and mid-infrared wavelengths can provideimportantand uniqueinformation aboutprotoplanetary disksaround young stars. In particular, infrared molecular spectroscopyisa good diagnostic of gas in theplanet-formingregionsofdisks within 10 AU of the star.Dataonthe physical conditions, gas content, structure,and chemistry of innerdisks canbeobtained through theanalysis of velocity-resolved line profiles

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APA

Carr, J. S. (2006). High-Resolution Infrared Spectroscopy of Protoplanetary Disks. In High Resolution Infrared Spectroscopy in Astronomy (pp. 203–213). Springer-Verlag. https://doi.org/10.1007/10995082_31

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